Cosmology with dark energy decaying through its chemical-potential contribution

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dc.creatorBesprosvany, J.
dc.date2007-12-29
dc.date.accessioned2026-07-07T11:19:55Z
dc.date.available2026-07-07T11:19:55Z
dc.descriptionThe consideration of dark energy's quanta, required also by thermodynamics, introduces its chemical potential into the cosmological equations. Isolating its main contribution, we obtain solutions with dark energy decaying to matter or radiation. When dominant, their energy densities tend asymptotically to a constant ratio, explaining today's dark energy-dark matter coincidence, and in agreement with supernova redshift data.
dc.description7 pages; presented at 2nd International Conference on Quantum Theories and Renormalization Group in Gravity and Cosmology, Barcelona, July, 2006
dc.identifierhttps://arxiv.org/abs/0801.0025
dc.identifierhttp://arxiv.org/abs/0801.0025
dc.identifierJ.Phys.A40:7099-7104,2007
dc.identifierdoi:10.1088/1751-8113/40/25/S68
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193853
dc.subjectAstrophysics
dc.titleCosmology with dark energy decaying through its chemical-potential contribution
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